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Binaries with Compact Components: Theoretical and Observational Challenges

Published online by Cambridge University Press:  22 February 2018

Ph. Podsiadlowski ,
S. Rappaport  and
E. Pfahl
Ph. Podsiadlowski
Affiliation:
Dep. of Astrophysics, University of Oxford, Oxford, OX1 3RH, UK
S. Rappaport
Affiliation:
Center for Space Research, M.I.T., Cambridge, MA 02139USA
E. Pfahl
Affiliation:
Center for Astrophysics, Cambridge, MA 02138USA

Abstract

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We report on recent progress in our theoretical understanding of X-ray binaries, which has largely been driven by new observations, and illustrate the interplay between theory and observations considering as examples intermediate-mass X-ray binaries, irradiation-driven evolution, ultraluminous X-ray sources and neutron stars with low-velocity kicks.

Resumen

Resumen

Presentamos una revisión sobre el reciente progreso teórico realizado en nuestra comprensión de binarias de rayos X, promovido en su mayoría, pоr nuevas observaciones y que ilustra la acción recíproca entre teoría y observaciones, considerando como ejemplos binarias de rayos X de masa intermedia, evolución impulsada por irradiación, fuentes de rayos X ultraluminosas y estrellas de neutrones con impulsos de baja velocidad.

Keywords

BinariesClose — Black Hole Physics — StarsNeutron — X-RaysStars
Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004 , pp. 97 - 100
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

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